We thank the reviewers for their useful comments, which greatly improved this article.
[-15]M.R. acknowledges support from the Narodowe Centrum Nauki (UMO-2020/38/E/ST9/00077). G.C.J. acknowledges ERC Advanced Grant 695671 “QUENCH” and support by the Science and Technology Facilities Council (STFC). YK acknowledges the support by funding from the European Research Council Advanced Grant ERC–2010–AdG–268107–EARLY.
This paper makes use of the following ALMA data: ADS/JAO.ALMA#2017.1.00428.L. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ.
This research made use of Astropy (http://www.astropy.org, accessed on May 31, 2022), a community-developed core Python package for Astronomy [1]}, [2]}.
We would also like to recognize the contributions from all of the members of the COSMOS Team who helped in obtaining and reducing the large amount of multiwavelength data that are now publicly available through IRSA at http://irsa.ipac.caltech.edu/Missions/cosmos.
html, accessed on May 31, 2022.
This article is dedicated to the memory of Olivier Le Fèvre, PI of the ALPINE survey.
